For an inviscid fluid of constant mass density with no body force, the Euler equations for an inviscid fluid areThe vector identityand irrotational flow give . Writing in terms of a velocity potential, we obtainThus the bracket depends only on time:Since adding a function of time to leaves unchanged, that function may be chosen to absorb . This is the Unsteady Bernoulli equation.
A radially symmetric velocity potential has . The incompressible flow condition in two-dimensional polar coordinates isso . The kinematic boundary condition at the bubble surface gives , henceAt the outer interface, . ThereforeandThe area of the incompressible liquid is conserved. These formulas are the radially symmetric incompressible flow in a planar annulus.
Apply the Unsteady Bernoulli equation at and and subtract, thereby eliminating its time-dependent constant. For and ,where each partial derivative is taken at fixed . Since and ,Equivalently, . This is the pressure in radially symmetric annular potential flow.
Let be the outer radius when . The area relation from part (i) givessoMoreover,The term in the pressure is second order, while the logarithm multiplying may be evaluated at equilibrium. The linearization is therefore
Per unit depth, the bubble volume is its area . At equilibrium its pressure equals , so . HenceContinuity of fluid pressure at the interface gives . Consequently
Equating the two linearized expressions for from parts (iii) and (iv) givesThis is the equation of simple harmonic motion. Thus the bubble performs small oscillations with angular frequencyThis is the small oscillation of a planar gas bubble in an annular liquid.
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